HD 12402

Summary

HD 12402 is a high proper-motion star^[1].

Key Facts

• HD 12402's instance of is recorded as high proper-motion star^[2].
• HD 12402's spectral class is recorded as K1III^[3].
• HD 12402's catalog code is recorded as HD 12402^[4].
• HD 12402's catalog code is recorded as GCRV 1117^[5].
• HD 12402's catalog code is recorded as GSC 01763-03030^[6].
• HD 12402's catalog code is recorded as HIC 9493^[7].
• HD 12402's catalog code is recorded as HIP 9493^[8].
• HD 12402's catalog code is recorded as IRAS 01592+2809^[9].
• HD 12402's catalog code is recorded as 2MASS J02020789+2824009^[10].
• HD 12402's catalog code is recorded as PPM 91301^[11].
• HD 12402's catalog code is recorded as SAO 75100^[12].
• HD 12402's catalog code is recorded as YZ 28 1102^[13].
• HD 12402's catalog code is recorded as AG+28 221^[14].
• HD 12402's catalog code is recorded as BD+27 320^[15].
• HD 12402's catalog code is recorded as TYC 1763-3030-1^[16].
• HD 12402's catalog code is recorded as Gaia DR1 299807615117390464^[17].
• HD 12402's catalog code is recorded as WEB 1991^[18].
• HD 12402's catalog code is recorded as Gaia DR2 299807619412692224^[19].
• HD 12402's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.594'}^[20].
• HD 12402's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.560'}^[21].
• HD 12402's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.2951'}^[22].
• HD 12402's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.150'}^[23].
• HD 12402's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.512'}^[24].
• HD 12402's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.274'}^[25].
• HD 12402's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.4805'}^[26].

Body

Designation and Status

HD 12402's instance of is recorded as high proper-motion star^[2].

History and Context

Catalog codes include HD 12402^[4], GCRV 1117^[5], GSC 01763-03030^[6], HIC 9493^[7], HIP 9493^[8], and IRAS 01592+2809^[9].